The following information shows the result of the orbit fit based on Gary Bernstein's method. Most of the information should be self-explanatory. Take special note that while the original Bernstein software works with barycentric coordinates, we convert these results into a heliocentric coordinate system.
# Object: 13TE187 # Created Wed May 8 01:15:22 2024 # Orbit generated from Bernstein formalism # Fitting 33 observations of 33 # Arc: 3.95y # First observation: 2013/10/13 # Last observation: 2017/09/24 Preliminary a, adot, b, bdot, g, gdot: 0.000035 0.020113 -0.000003 0.000199 0.022290 0.000000 # Chi-squared of fit: 6.87 DOF: 60 RMS: 0.08 # Min/Max residuals: -0.25 0.16 # Exact a, adot, b, bdot, g, gdot: 1.472436E-05 2.004185E-02 1.607892E-07 1.976571E-04 2.214446E-02 -1.506875E-03 # Covariance matrix: 1.6593E-13 -4.9533E-14 -8.8695E-16 1.6941E-16 1.0628E-13 8.9281E-14 -4.9533E-14 2.2366E-13 -1.9149E-15 2.5779E-15 1.7587E-13 2.9527E-12 -8.8695E-16 -1.9149E-15 1.2635E-13 -4.0401E-14 -4.4868E-15 -3.3261E-14 1.6941E-16 2.5779E-15 -4.0401E-14 1.9936E-14 3.0561E-15 3.8973E-14 1.0628E-13 1.7587E-13 -4.4868E-15 3.0561E-15 4.8436E-13 3.1953E-12 8.9281E-14 2.9527E-12 -3.3261E-14 3.8973E-14 3.1953E-12 4.4044E-11 # lat0 lon0 xBary yBary zBary JD0 -2.475517 11.593919 -0.139496 -0.042541 -0.986697 2456578.646678 # Heliocentric elements and errors Epoch: 2456570.5000 = 2013/10/05 Mean Anomaly: 247.91488 +/- 0.145 Argument of Peri: 43.81838 +/- 0.133 Long of Asc Node: 88.44905 +/- 0.009 Inclination: 2.48948 +/- 0.000 Eccentricity: 0.08296935 +/- 0.0003 Semi-Major Axis: 44.50768476 +/- 0.0057 Time of Perihelion: 2490337.8042 +/- 43.2 Perihelion: 40.81491124 +/- 0.0130 Aphelion: 48.20045828 +/- 0.0134 Period (y) 296.9345 +/- 0.06 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 45.13415139 +/- 0.0014 Ecliptic Y 9.40532820 +/- 0.0003 Ecliptic Z -1.95051413 +/- 0.0001 Ecliptic XDOT -0.00068546 +/- 0.0000 Ecliptic YDOT 0.00238869 +/- 0.0000 Ecliptic ZDOT 0.00003260 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 46.14494908 +/- 0.0014 Geocenter to KBO 45.15801284 +/- 0.0014 # Hcoef: 6.48
The following table shows the complete astrometric record for 13TE187. The first three columns show the date of observation. The next six columns are RA and DEC. The next column (when provided) is the observed magnitude and filter. The next column is the object name (13TE187) followed by the observatory code and reference code for the source of the astrometry.
2013 10 13.14590 00 46 30.798 +02 18 22.32 22.9i 13TE187 W84 C~4yRC 2013 10 13.14590 00 46 30.80 +02 18 22.3 23.0i 13TE187 W84 C~3clP 2013 10 13.14731 00 46 30.799 +02 18 22.41 22.4z 13TE187 W84 C~4yRC 2013 10 13.14731 00 46 30.80 +02 18 22.4 22.5z 13TE187 W84 C~3clP 2013 11 22.10101 00 44 11.152 +02 04 50.28 23.2r 13TE187 W84 C~4yRC 2013 11 22.10101 00 44 11.15 +02 04 50.3 23.3r 13TE187 W84 C~3clP 2013 11 22.10256 00 44 11.149 +02 04 50.10 22.8i 13TE187 W84 C~4yRC 2013 11 22.10256 00 44 11.15 +02 04 50.1 22.9i 13TE187 W84 C~3clP 2013 11 22.14496 00 44 11.028 +02 04 49.52 22.2z 13TE187 W84 C~4yRC 2013 11 22.14496 00 44 11.03 +02 04 49.5 22.4z 13TE187 W84 C~3clP 2014 10 21.23370 00 50 12.119 +02 42 37.04 23.2r 13TE187 W84 C~4yRC 2014 10 21.23370 00 50 12.12 +02 42 37.0 23.3r 13TE187 W84 C~3clP 2014 11 14.06558 00 48 45.943 +02 34 15.83 22.9r 13TE187 W84 C~4yRC 2014 11 14.06558 00 48 45.94 +02 34 15.8 23.1r 13TE187 W84 C~3clP 2016 09 01.36467 01 01 52.809 +03 57 59.43 23.4i 13TE187 W84 C~4yRC 2016 09 01.36467 01 01 52.81 +03 57 59.4 23.3i 13TE187 W84 C~3clP 2016 09 01.36604 01 01 52.796 +03 57 59.30 23.5r 13TE187 W84 C~4yRC 2016 09 01.36604 01 01 52.80 +03 57 59.3 23.6r 13TE187 W84 C~3clP 2016 09 01.36741 01 01 52.816 +03 57 59.26 24.2g 13TE187 W84 C~4yRC 2016 11 05.16584 00 57 40.446 +03 31 42.42 23.1r 13TE187 W84 C~4yRC 2016 11 05.16584 00 57 40.45 +03 31 42.4 23.0r 13TE187 W84 C~3clP 2016 11 05.16722 00 57 40.438 +03 31 42.33 22.8i 13TE187 W84 C~4yRC 2016 11 05.16722 00 57 40.44 +03 31 42.3 22.8i 13TE187 W84 C~3clP 2016 11 05.16861 00 57 40.433 +03 31 42.52 24.3g 13TE187 W84 C~4yRC 2016 11 06.16691 00 57 36.822 +03 31 21.69 22.0z 13TE187 W84 C~4yRC 2016 11 06.16691 00 57 36.83 +03 31 21.8 22.6z 13TE187 W84 C~3clP 2016 11 18.08956 00 56 57.502 +03 27 42.89 22.5i 13TE187 W84 C~4yRC 2016 11 18.08956 00 56 57.50 +03 27 42.9 22.5i 13TE187 W84 C~3clP 2017 08 28.28676 01 06 20.672 +04 26 48.20 23.2r 13TE187 W84 C~4yRC 2017 09 14.32230 01 05 24.513 +04 20 31.42 23.1i 13TE187 W84 C~4yRC 2017 09 18.30613 01 05 09.566 +04 18 54.11 23.2r 13TE187 W84 C~4yRC 2017 09 18.30750 01 05 09.559 +04 18 54.05 23.4g 13TE187 W84 C~4yRC 2017 09 24.29119 01 04 46.163 +04 16 23.87 22.3z 13TE187 W84 C~4yRC
The following table shows the residuals to the orbit fit. The first coumn is the point number. The second column is the time, in years, measured from the first observation. The third and fifth columns are the regularized positions used in the orbit fit. The fourth and sixth columns are the residuals, in arc seconds, for RA and Dec respectively.
1 0.0000 0.00 -0.09 0.00 -0.00
2 0.0000 0.02 -0.07 -0.03 -0.03
3 0.0000 0.05 0.06 0.08 0.07
4 0.0000 0.06 0.07 0.06 0.06
5 0.1094 -2244.18 0.07 68.98 0.11
6 0.1094 -2244.20 0.05 69.01 0.14
7 0.1094 -2244.28 0.03 68.83 -0.05
8 0.1094 -2244.29 0.02 68.83 -0.04
9 0.1095 -2246.17 -0.12 68.98 -0.03
10 0.1095 -2246.19 -0.14 69.01 0.00
11 1.0215 3621.69 0.07 47.34 -0.13
12 1.0215 3621.70 0.08 47.38 -0.09
13 1.0867 2236.84 0.00 88.63 -0.01
14 1.0867 2236.90 0.05 88.64 -0.00
15 2.8863 15073.09 -0.01 144.12 0.02
16 2.8863 15073.09 -0.01 144.09 -0.01
17 2.8863 15072.91 -0.12 144.05 -0.04
18 2.8863 15072.86 -0.17 144.07 -0.02
19 2.8863 15073.12 0.16 143.92 -0.17
20 3.0637 10963.39 0.11 152.39 -0.04
21 3.0637 10963.34 0.06 152.43 -0.00
22 3.0637 10963.21 0.01 152.36 -0.08
23 3.0637 10963.19 -0.00 152.40 -0.04
24 3.0637 10963.20 0.09 152.60 0.16
25 3.0665 10905.28 -0.09 154.42 0.04
26 3.0665 10905.12 -0.25 154.36 -0.01
27 3.0991 10275.96 -0.00 181.02 0.03
28 3.0991 10275.98 0.02 181.00 0.00
29 3.8744 19467.70 0.08 192.73 0.10
30 3.9211 18539.65 0.11 168.64 0.12
31 3.9320 18293.91 -0.01 165.04 0.00
32 3.9320 18293.79 -0.04 165.03 -0.01
33 3.9484 17910.05 -0.05 161.42 -0.02
The following table comes from a 10My integration of the orbit of the object. Three columns are shown. The first column is the result of integrating the nominal orbit. The other two columns are based on clones of the nominal orbit that are +/- 3 sigma from the nominal orbit. If all three types agree then the classificiation is deemed secure. The basis for these calculations is described in more detail in AJ, 129, 1117 (2005). Any use made of these calculations should refer to and credit this publication and the Deep Ecliptic Survey Team.
13TE187 quality flag:3 Type: CLASSICAL CLASSICAL CLASSICAL axisobj 44.750 44.767 44.734 ecceobj 0.078 0.079 0.078 incobj 2.490 2.490 2.490 qmin 39.693 39.232 39.800 qmax 49.544 50.272 49.506 amean 44.505 44.557 44.488 amin 44.134 44.157 44.127 amax 44.902 44.980 44.869 emean 0.088 0.092 0.087 emin 0.070 0.071 0.070 emax 0.104 0.118 0.103 imean 0.948 0.888 0.961 imin 0.163 0.103 0.161 imax 1.488 1.498 1.510 excite_mean 0.090 0.094 0.089 fracstop 1.000 1.000 1.000 cjmean 3.098 3.097 3.098 libcent 0 -180.0 -180.0 183.0 libamp 0 -180.0 -180.0 162.1 libcent 1 -180.0 -180.0 -180.0 libamp 1 -180.0 -180.0 -180.0 libcent 2 -180.0 -180.0 -180.0 libamp 2 -180.0 -180.0 -180.0 libcent 3 -180.0 -180.0 -180.0 libamp 3 -180.0 -180.0 -180.0 libcent 4 -180.0 -180.0 -180.0 libamp 4 -180.0 -180.0 -180.0 kozaimean 177.5 194.7 176.9 kozaiamp 179.9 180.0 180.0